Constraints on type ia supernovae from near infrared spectra
We describe a research program to improve the understanding of Type IaSupernovae (SNe Ia) by modeling and observing near infrared (NIR) spectra ofthese events. The NIR between 0.9 and 2.5 is optimal for examining certainproducts of the SNe Ia explosion that may be blended or obscured in other spectr...
Shranjeno v:
| izdano v: | Revista Mexicana de Astronomía y Astrofísica |
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| Principais autores: | , , |
| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
Universidad Nacional Autónoma de México
2001
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| Teme: | |
| Online dostop: | https://www.redalyc.org/articulo.oa?id=57101042 |
| Oznake: |
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